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Constancy of period in TX Ceti

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dc.contributor.author Srivastava, R. K.
dc.date.accessioned 2010-02-02T06:51:24Z
dc.date.available 2010-02-02T06:51:24Z
dc.date.issued 1990
dc.identifier.citation This article downloded from ADS Free Online Journal en_US
dc.identifier.uri http://hdl.handle.net/123456789/483
dc.description.abstract A slightly improved period (P = 0.ᵈ7408401) of the eclipsing binary system TX Ceti has been given, which is based on all available times of minima. The O-C diagrams based on the period given in PPEN (1980) and based on the new period, have been given. The period of TX Ceti shows fair constancy between the time interval 1928 to 1988. The present O-C diagrams do not confirm, either the presence of a third body or the presence of mass transfer as suggested earlier. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries ass166-205
dc.subject TX Ceti en_US
dc.title Constancy of period in TX Ceti en_US
dc.type Article en_US


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